{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:DQMUPX6CKEFTUSCNN3VOMCJIHK","short_pith_number":"pith:DQMUPX6C","schema_version":"1.0","canonical_sha256":"1c1947dfc2510b3a484d6eeae609283a827db8fdd2beb0652b633fa3006243e4","source":{"kind":"arxiv","id":"1705.00592","version":2},"attestation_state":"computed","paper":{"title":"A Radiative Neutrino Mass Model with SIMP Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Koji Tsumura, Shu-Yu Ho, Takashi Toma","submitted_at":"2017-05-01T16:59:02Z","abstract_excerpt":"We propose the first viable radiative seesaw model, in which the neutrino masses are induced radiatively via the two-loop Feynman diagram involving Strongly Interacting Massive Particles (SIMP). The stability of SIMP dark matter (DM) is ensured by a $\\mathbb{Z}_5$ discrete symmetry, through which the DM annihilation rate is dominated by the $3 \\to 2$ self-annihilating processes. The right amount of thermal relic abundance can be obtained with perturbative couplings in the resonant SIMP scenario, while the astrophysical bounds inferred from the Bullet cluster and spherical halo shapes can be sa"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1705.00592","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-05-01T16:59:02Z","cross_cats_sorted":[],"title_canon_sha256":"89e2e6923d3d0f6ad3d1a0565ec1ff1768806617f75b9e924f25d825f2ca710f","abstract_canon_sha256":"9ee1cd6c07eb975cd36d9620599c5918cad9973ccd7107f3bd216da72fc07c04"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:39:22.633556Z","signature_b64":"sr9yZKyGQSf4X7OIhfWAEfaJwHo7HpJtOoRshZB+bUaWtQJqvV8V3yavEXO/zUflK/weC1iAtvj/3sCksuKtBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1c1947dfc2510b3a484d6eeae609283a827db8fdd2beb0652b633fa3006243e4","last_reissued_at":"2026-05-18T00:39:22.632801Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:39:22.632801Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Radiative Neutrino Mass Model with SIMP Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Koji Tsumura, Shu-Yu Ho, Takashi Toma","submitted_at":"2017-05-01T16:59:02Z","abstract_excerpt":"We propose the first viable radiative seesaw model, in which the neutrino masses are induced radiatively via the two-loop Feynman diagram involving Strongly Interacting Massive Particles (SIMP). The stability of SIMP dark matter (DM) is ensured by a $\\mathbb{Z}_5$ discrete symmetry, through which the DM annihilation rate is dominated by the $3 \\to 2$ self-annihilating processes. The right amount of thermal relic abundance can be obtained with perturbative couplings in the resonant SIMP scenario, while the astrophysical bounds inferred from the Bullet cluster and spherical halo shapes can be sa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.00592","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1705.00592","created_at":"2026-05-18T00:39:22.632918+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.00592v2","created_at":"2026-05-18T00:39:22.632918+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.00592","created_at":"2026-05-18T00:39:22.632918+00:00"},{"alias_kind":"pith_short_12","alias_value":"DQMUPX6CKEFT","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_16","alias_value":"DQMUPX6CKEFTUSCN","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_8","alias_value":"DQMUPX6C","created_at":"2026-05-18T12:31:12.930513+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2506.12642","citing_title":"Dark matter spikes with strongly self-interacting particles","ref_index":29,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DQMUPX6CKEFTUSCNN3VOMCJIHK","json":"https://pith.science/pith/DQMUPX6CKEFTUSCNN3VOMCJIHK.json","graph_json":"https://pith.science/api/pith-number/DQMUPX6CKEFTUSCNN3VOMCJIHK/graph.json","events_json":"https://pith.science/api/pith-number/DQMUPX6CKEFTUSCNN3VOMCJIHK/events.json","paper":"https://pith.science/paper/DQMUPX6C"},"agent_actions":{"view_html":"https://pith.science/pith/DQMUPX6CKEFTUSCNN3VOMCJIHK","download_json":"https://pith.science/pith/DQMUPX6CKEFTUSCNN3VOMCJIHK.json","view_paper":"https://pith.science/paper/DQMUPX6C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.00592&json=true","fetch_graph":"https://pith.science/api/pith-number/DQMUPX6CKEFTUSCNN3VOMCJIHK/graph.json","fetch_events":"https://pith.science/api/pith-number/DQMUPX6CKEFTUSCNN3VOMCJIHK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DQMUPX6CKEFTUSCNN3VOMCJIHK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DQMUPX6CKEFTUSCNN3VOMCJIHK/action/storage_attestation","attest_author":"https://pith.science/pith/DQMUPX6CKEFTUSCNN3VOMCJIHK/action/author_attestation","sign_citation":"https://pith.science/pith/DQMUPX6CKEFTUSCNN3VOMCJIHK/action/citation_signature","submit_replication":"https://pith.science/pith/DQMUPX6CKEFTUSCNN3VOMCJIHK/action/replication_record"}},"created_at":"2026-05-18T00:39:22.632918+00:00","updated_at":"2026-05-18T00:39:22.632918+00:00"}